Abstract
Properties of solar-flare EUV flashes measured via a type of ionospheric event, called a sudden frequency deviation (SFD), are presented. SFD's are sensitive to bursts of radiation in the 1–1030 Å wavelength range. He ii 303.8 Å, O v 629.7 Å, HL γ 972.5 Å and C iii 977.0 Å have essentially the same impulsive time dependence as the 1–1030 Å flash responsible for SFD's. Soft X-rays (2–20 Å) and certain EUV lines have a much slower time dependence than the 1–1030 Å flash. Most SFD's have some fine structure, but marked quasi-periodicity in EUV flashes is quite rare. EUV flashes are closely associated with hard X-ray bursts, white-light emission, microwave radio bursts and small bright impulsive kernels in the Hα flare. The intensity of EUV flashes depends on the central meridian distance of the Hα flare location; the intensity decreases at the limb. The total energy radiated in the 10–1030 Å flash for the largest events observed is about 1031 ergs.
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Donnelly, R.F. Extreme ultraviolet flashes of solar flares observed via sudden frequency deviations: Experimental results. Sol Phys 20, 188–203 (1971). https://doi.org/10.1007/BF00146110
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DOI: https://doi.org/10.1007/BF00146110